M. Laneuville

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About

M. Laneuville is a planetary scientist whose research focuses on the thermal and magmatic evolution of terrestrial bodies, with a particular emphasis on the Moon and Mars. Their major contributions include advancing our understanding of post-differentiation magmatism—the volcanic and intrusive activity that occurs after a planet's initial core and crust formation. Laneuville's most cited work, "Magmatic Evolution II: A New View of Post-Differentiation Magmatism" (2023, 42 citations), co-authored with Charles Shearer, challenges traditional models by proposing that prolonged, low-degree melting can sustain magmatic activity for billions of years after a body's primary differentiation. This work has reshaped how scientists interpret the duration and style of volcanism on the Moon, linking geophysical models with geochemical observations. Laneuville's research has been instrumental in reconciling thermal history models with the surprising longevity of lunar volcanism revealed by sample analyses and remote sensing. Their contributions have been recognized through collaborations with leading institutions like the Institute of Meteoritics and the Lunar & Planetary Institute, and their work continues to influence the design of future planetary exploration missions.